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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-01-27T03:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-01-27T03:36:00-CME-001 (version 2)
Note Keyword:
DFL: Likely deflection of the event within the FOV
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: CME visible in the north of SOHO LASCO C2/C3 and STEREO A COR2. The source is believed to be on the far side, and material is seen lifting off beyond the limb, towards the west, in GOES SUVI 304 around 2024-01-27T03:09Z. Moving field lines can be seen rising beyond the NW limb in SDO AIA 171. This is not clearly visible in STEREO A EUV 195 imagery. This CME may deflect in the field of view, as the bulk of the CME appears to move east of the source. Overlaps in the field of view of the coronagraphs with CME: 2024-01-27T04:24Z.

Submitted on 2024-01-27T17:10Z by Mary Aronne

A Notification with ID 20240127-AL-001 was sent on 2024-01-27T15:25Z

The List of CME Analysis already entered:
Event Type Catalog
Measurement TypeCME measurement type: Leading Edge (LE), Shock Front (SH), Right Hand Boundary (RHB), Left Hand Boundary (LHB), Black/White Boundary (BW), Prominence Core (COR), Disconnection Front (DIS), Trailing Edge (TE).
Prime?"primary flag" which is either True or False. If there are multiple CME analysis entries for a single CME, this flag would indicate which analysis is considered most accurate per measurement type. This is a helpful flag if you would like to download only one most accurate CME analysis per CME per Measurement Type
 Technique Long Lat Speed Type Half Width Time 21.5 Note WSA-ENLIL+Cone Result(s) Submitted By
CME Analysis M2M_CATALOG LE true SWPC_CAT -175.0 51.0 534.0 C 30.0 2024-01-27T09:49Z This measurement is based on the best fit in SWPC_CAT between SOHO LASCO C2/C3 and STEREO A COR2. Similar parameters were derived in StereoCAT. Because this measurement is approximate, the longitude may vary by +/- 10 degrees. 1: Result 1 (2.0 AU)
Parker Solar Probe = 2024-01-29T18:19Z
Mary Aronne on 2024-01-27T14:53Z



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